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If the number of views is not sufficient, star-shaped artifacts (streak artifacts) could arise in cross-sectional images. Therefore, we estimated the point spread function (PSF) of cross-sectional Compton images and the effect of the number of views by Monte Carlo simulations and experimental studies. \nMaterials and Methods: A cross-sectional Compton image was reconstructed using a dataset comprising 719 view directions and PSF was analyzed using a radial distribution. The peak height, full width at half maximum (FWHM), background (BG), and residual sum of squares (RSS) were calculated from the obtained PSF. In addition, RSSs were plotted against the number of views to estimate the required number to suppress star-shaped artifacts. \nResults: There was no correlation found between the number of views and both FWHM (16 mm) and peak/BG ratio (~1×10^4). RSSs were reduced with the number of views and approached the minimum asymptotically. 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Effect of number of views on cross-sectional Compton imaging: A fundamental study with backprojection
https://repo.qst.go.jp/records/49337
https://repo.qst.go.jp/records/49337c016710a-413e-46ea-8c77-7029e52f5e5f
Item type | 学術雑誌論文 / Journal Article(1) | |||||
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公開日 | 2018-12-18 | |||||
タイトル | ||||||
タイトル | Effect of number of views on cross-sectional Compton imaging: A fundamental study with backprojection | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | journal article | |||||
アクセス権 | ||||||
アクセス権 | metadata only access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
著者 |
Sakai, Makoto
× Sakai, Makoto× Raj, kumar Parajuli× Kikuchi, Mikiko× Yamaguchi, Mitsutaka× Nagao, Yuto× Kawachi, Naoki× Arakawa, Kazuo× Nakano, (Gunma Univ.) Takashi× 酒井 真理× ラジュ クマル パラジュリ× 菊地 美貴子× 山口 充孝× 長尾 悠人× 河地 有木× 荒川 和夫 |
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抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | Introduction: We have been developing a medical imaging technique using a Compton camera, which is expected to reconstruct three-dimensional images. If the number of views is not sufficient, star-shaped artifacts (streak artifacts) could arise in cross-sectional images. Therefore, we estimated the point spread function (PSF) of cross-sectional Compton images and the effect of the number of views by Monte Carlo simulations and experimental studies. Materials and Methods: A cross-sectional Compton image was reconstructed using a dataset comprising 719 view directions and PSF was analyzed using a radial distribution. The peak height, full width at half maximum (FWHM), background (BG), and residual sum of squares (RSS) were calculated from the obtained PSF. In addition, RSSs were plotted against the number of views to estimate the required number to suppress star-shaped artifacts. Results: There was no correlation found between the number of views and both FWHM (16 mm) and peak/BG ratio (~1×10^4). RSSs were reduced with the number of views and approached the minimum asymptotically. Correlation was observed between the required number of views and the number of Compton events used for image reconstruction. Conclusion: We determined the PSF of cross-sectional Compton images and the effect of the number of views on the images. The required number of views to suppress the star-shaped artifact is related to the square root of the number of Compton events used to reconstruct the image. From this study, we concluded that 21 or more views are required for clinical purposes. |
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書誌情報 |
Physica Medica 巻 56, p. 1-9, 発行日 2018-11 |
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出版者 | ||||||
出版者 | Elsevier | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 1120-1797 | |||||
DOI | ||||||
識別子タイプ | DOI | |||||
関連識別子 | 10.1016/j.ejmp.2018.11.006 | |||||
関連サイト | ||||||
識別子タイプ | DOI | |||||
関連識別子 | https://doi.org/10.1016/j.ejmp.2018.11.006 | |||||
関連名称 | https://doi.org/10.1016/j.ejmp.2018.11.006 |